The Stromvil Seven-Colour Photometric System for GAIA

Details The Stromvil Seven-Colour Photometric System for GAIA The Stromvil Seven-Colour Photometric System for GAIA

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997esasp.402..761s&link_type=abstract

Proceedings of the ESA Symposium `Hipparcos - Venice '97', 13-16 May, Venice, Italy, ESA SP-402 (July 1997), p. 761-766

Physics

6

Scientific paper

In our previous publications it was shown that the Stromvil seven-colour photometric system, when set up on a GAIA-type satellite, will be able to classify stars of all normal spectral classes down to 16 mag. In the present paper we demonstrate that the same system makes possible the photometric identification of a number of peculiar types of stars, including emission-line stars, metallic-line A and F stars, chemically peculiar B and A stars, metal-deficient F-G-K dwarfs (subdwarfs), metal-deficient G and K giants, blue horizontal-branch stars, white dwarfs and carbon-rich stars.

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